Kinetic Alfvén wave explanation of the Hall fields in magnetic reconnection-Reference-Cited by-同舟云学术

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Kinetic Alfvén wave explanation of the Hall fields in magnetic reconnection

Published:2017-01-25 Issue:2 Volume:44 Page:634-640
ISSN:0094-8276
Container-title:Geophysical Research Letters
language:en
Short-container-title:Geophys. Res. Lett.

Author:

Dai Lei¹^ORCID,Wang Chi¹^ORCID,Zhang Yongcun¹^ORCID,Lavraud Benoit²^ORCID,Burch James³^ORCID,Pollock Craig⁴^ORCID,Torbert Roy B.⁵^ORCID

Affiliation:

1. State Key Laboratory of Space Weather, National Space Science CenterChinese Academy of Sciences Beijing China

2. Institut de Recherche en Astrophysique et PlanétologieUniversité de Toulouse Toulouse France

3. Southwest Research Institute San Antonio Texas USA

4. NASA Goddard Space Flight Center Greenbelt Maryland USA

5. University of New Hampshire Durham New Hampshire USA

Funder

NNSFC

Specialized Research Fund for State Key Laboratories of China

Publisher

American Geophysical Union (AGU)

Subject

General Earth and Planetary Sciences,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1002/2016GL071044

Reference46 articles.

1. Geospace Environmental Modeling (GEM) Magnetic Reconnection Challenge

2. Magnetic reconnection at the dayside magnetopause: Advances with MMS

3. Magnetospheric Multiscale Overview and Science Objectives

4. Electron-scale measurements of magnetic reconnection in space

5. Momentum transport near a magnetic X line in collisionless reconnection

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